ESSENTIAL COSMIC PERS.-W/MASTER.ACCESS
9th Edition
ISBN: 9780135795750
Author: Bennett
Publisher: PEARSON
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Chapter 13, Problem 26EAP
To determine
Whether the given statement makes sense or not.
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QUESTION 16
Use the figure shown below to complete the following statement: A low-mass protostar (0.5 to 8M the mass compared to our sun) remains roughly constant in
decreases in
until it makes a turn towards the main sequence, as it follows its evolutionary track.
Protostars of different masses follow diferent
paths on their way to the main sequence.
107
Luminosity (L)
10
105
10
107
10²
101
1
10-1
10-2
10-3
Spectral
type
0.01 R
0.001
Re
60 M
MAIN SEQUENCE
40,000 30,000
20 Mau
10 Mgun
5 Mun
0.1 Run
Ren
radius; temperature
luminosity; radius
3 Min.
05 BO
temperature; luminosity
Oluminosity: temperature
radius: luminosity
1 M
10,000 6000
Surlace temperature (K)
1,000 Rs
2 M STAR
L
0.8 M
B5 AO FOGO КБ МБ
-10
+10
3000
Absolute visual magnitude
and
Most stars (Main sequence) generate light
through the same mechanism. Because of this,
there is an empirical relation between their
mass, M, and their Luminosity, L. This relation
could be written in the form
L/Lsun = (M/Msun,
This relation is shown in the log-log diagram
below. Find the value of a and round it to the
nearest integer.
10
104
102
10-2
10-4
0.1
1.0
2.0
0.2
0.5
5.0
10.0
20.0
Mam (solar masses)
Luminosty (solar units)
Life on Earth wouldn't be possible without supernovae. Why?
Chapter 13 Solutions
ESSENTIAL COSMIC PERS.-W/MASTER.ACCESS
Ch. 13 - Prob. 1VSCCh. 13 - Prob. 2VSCCh. 13 - Prob. 3VSCCh. 13 - Prob. 4VSCCh. 13 - Prob. 1EAPCh. 13 - Prob. 2EAPCh. 13 - Prob. 3EAPCh. 13 - Prob. 4EAPCh. 13 - Prob. 5EAPCh. 13 - Prob. 6EAP
Ch. 13 - Prob. 7EAPCh. 13 - Prob. 8EAPCh. 13 - Prob. 9EAPCh. 13 - Prob. 10EAPCh. 13 - Prob. 11EAPCh. 13 - Prob. 12EAPCh. 13 - Prob. 13EAPCh. 13 - Prob. 14EAPCh. 13 - Prob. 15EAPCh. 13 - Prob. 16EAPCh. 13 - Prob. 17EAPCh. 13 - Prob. 18EAPCh. 13 - Prob. 19EAPCh. 13 - Prob. 20EAPCh. 13 - Prob. 21EAPCh. 13 - Prob. 22EAPCh. 13 - Prob. 23EAPCh. 13 - Prob. 24EAPCh. 13 - Prob. 25EAPCh. 13 - Prob. 26EAPCh. 13 - Prob. 27EAPCh. 13 - Prob. 28EAPCh. 13 - Prob. 29EAPCh. 13 - Prob. 30EAPCh. 13 - Prob. 31EAPCh. 13 - Prob. 32EAPCh. 13 - Prob. 33EAPCh. 13 - Prob. 34EAPCh. 13 - Prob. 35EAPCh. 13 - Prob. 36EAPCh. 13 - Prob. 37EAPCh. 13 - Prob. 39EAPCh. 13 - Prob. 40EAPCh. 13 - Prob. 41EAPCh. 13 - Prob. 42EAPCh. 13 - Prob. 43EAPCh. 13 - Prob. 44EAPCh. 13 - Prob. 45EAPCh. 13 - Prob. 46EAPCh. 13 - Prob. 48EAPCh. 13 - Prob. 49EAPCh. 13 - Prob. 50EAPCh. 13 - Prob. 51EAPCh. 13 - Prob. 52EAPCh. 13 - Prob. 53EAP
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- Describe the forces acting on a star during the main sequence period of its life?arrow_forwardThe sun will eventually cease fusing nuclei in it interior and will then be dead what general term is used to describe dead but still illuminus stars when the star becomes such a star name two kinds of of nuclei that are expected to dominate its core as a result of the nuclear fusion that has taken place prior to its deatharrow_forwardThe hottest star in the Orion Nebula has a surface temperature of 40,000 K. At what wavelength does it radiate the most energy?arrow_forward
- Do you think that nuclear fusion takes place in the atmospheres of stars? Why or why not?arrow_forwardArrange the following stars in order of their evolution: A. A star with no nuclear reactions going on in the core, which is made primarily of carbon and oxygen. B. A star of uniform composition from center to surface; it contains hydrogen but has no nuclear reactions going on in the core. C. A star that is fusing hydrogen to form helium in its core. D. A star that is fusing helium to carbon in the core and hydrogen to helium in a shell around the core. E. A star that has no nuclear reactions going on in the core but is fusing hydrogen to form helium in a shell around the core.arrow_forwardFor a main sequence star with luminosity L, how many kilograms of hydrogen is being converted into helium per second? Use the formula that you derive to estimate the mass of hydrogen atoms that are converted into helium in the interior of the sun (LSun = 3.9 x 1026 W). (Note: the mass of a hydrogen atom is 1 mproton and the mass of a helium atom is 3.97 mproton. You need four hydrogen nuclei to form one helium nucleus.)arrow_forward
- Question 41 .Suppose you are looking at H-R diagrams of two similar star clusters. The most luminous main sequence stars in the Porcini cluster are much more luminous than the most luminous main sequence stars in the Morel cluster. What can you conclude? O the Porcini cluster is younger than the Morel cluster O the Porcini cluster is farther away than the Morel cluster O the Porcini cluster is lower in metallicity than the Morel cluster O the Porcini cluster is larger in diameter than the Morel clusterarrow_forwardWhat causes an aging giant star to produce a planetary nebula?arrow_forwardNuclear fusion occurs during most of a star's life O True O Falsearrow_forward
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